Comments on the optical counterpart of the X-ray source 3U 0352 + 30

Details Comments on the optical counterpart of the X-ray source 3U 0352 + 30 Comments on the optical counterpart of the X-ray source 3U 0352 + 30

Aug 1976

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1976apj...207l.185m&link_type=abstract

Astrophysical Journal, vol. 207, Aug. 1, 1976, pt. 2, p. L185-L187. Research supported by the Research Corp.;

Astronomy and Astrophysics

Astrophysics

1

Giant Stars, M Stars, X Ray Sources, Light Curve, Line Spectra, Stellar Spectrophotometry

Scientific paper

Spectral and photometric observations of ADS 2859 B, the faint companion
to X Per, show it to be a normal M giant rather than a T Tauri star as
previously reported in the literature. Consequently, there is no
substantive reason to associate it with the X-ray source 3U 0352 + 30. A
search for rapid light variations of X Per itself proved negative.

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